(480808) 1994 XL1 is a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Aten group, approximately 200 meters (700 feet) in diameter. It was discovered on 6 December 1994, by Scottish–Australian astronomer Robert McNaught at Siding Spring Observatory in Australia.[1] It was one of the first asteroids discovered to have a semi-major axis less than Venus.[citation needed]
Discovery[1][2] | |
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Discovered by | R. H. McNaught |
Discovery site | Siding Spring Obs. |
Discovery date | 6 December 1994 |
Designations | |
MPC designation | (480808) 1994 XL1 |
Alternative designations | 1994 XL1 |
Minor planet category | NEO · Aten · PHA[1][3] |
Orbital characteristics[3] | |
Epoch 30 January 2013 (JD 2456322.5) | |
Uncertainty parameter 0 | |
Observation arc | 21.99 yr (8,033 days) |
Aphelion | 1.0240 AU |
Perihelion | 0.3178 AU |
Semi-major axis | 0.6709 AU |
Eccentricity | 0.5263 |
Orbital period (sidereal) | 0.55 yr (201 days) |
Mean anomaly | 205.64° |
Mean motion | 1° 47m 36.96s / day |
Inclination | 28.167° |
Longitude of ascending node | 252.68° |
Argument of perihelion | 356.54° |
Earth MOID | 0.0365 AU · 14.2 LD |
Physical characteristics | |
Mean diameter | 0.2 km (est. at 0.20)[4] |
Absolute magnitude (H) | 20.9[3] |
1994 XL1 orbits the Sun at a distance of 0.3–1.0 AU once every 0 years and 7 months (201 days). Its orbit has an eccentricity of 0.53 and an inclination of 28° with respect to the ecliptic.[3] No precoveries were taken, and no prior identifications were made. The body's observation arc begins with its official discovery observation.[1]
The asteroid has an Earth minimum orbital intersection distance of 0.0365 AU (5,460,000 km), which translates into 14.2 lunar distances.[3] It passed 0.03709 AU (5,550,000 km) from Earth on 6 December 1994.[5] On 4 December 2044, it will pass again at 0.03637 AU (5,440,000 km) from Earth.[5]
1994 XL1 has not been observed by any of the space-based surveys such as the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission. Based on a generic magnitude-to-diameter conversion, 1994 XL1 measures approximately 0.2 kilometers in diameter assuming an albedo of 0.20, which is a typical value for stony S-type asteroids.[4]
As of 2017, no rotational lightcurve of this object has been obtained. The body's rotation period, shape and poles remain unknown.[6]
After its first observation in 1994, this minor planet was numbered 23 year later by the Minor Planet Center on 12 January 2017 (M.P.C. 112958),[7]: 698 after its last observation with the LCO–A 1-meter global telescope station at Sutherland, South Africa, on 6 December 2016 (K91). As of 2018, the asteroid has not been named .[1][3]
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